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Interactions between the Planetary Magnetic Field and the Surrounding Gas Flows in the Final Stage of the Giant Planet Formation. I. Two Distinct Evolutionary Scenarios

Authors: Pengfei Tang, Xiaogang Wang, Tianchun Zhou, Jiayong Zhong

Pengfei Tang et al 2026 The Astrophysical Journal 1005 .

Provider: AAS Journals

Caption: Figure 12.

Same as Figure 10, but for the inflating magnetosphere at ﹩t=0.6810\,{{\rm{\Omega }}}_{{\rm{KH}}}^{-1}﹩.

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